Exploring the origin and fate of the universe with radio and millimeter-wave instrumentation and observations

我的研究计划的主要重点是通过端到端的直接天体物理测量揭示宇宙的起源，命运和组成。我的团队开发的关键技术使新仪器成为可能，为一些最令人兴奋的宇宙时代打开了新的观测窗口。小组成员是使用这些仪器获得重要宇宙学结果的主要作者。 我的团队共同开发并共同建造了加拿大氢强度测绘实验（CHIME），这是一种新颖的新射电望远镜，于2017年秋季首次亮相。我们一直是CHIME仪器设计和实现的核心，负责GHz数字化仪和基于FPGA的相关器，并指导整个项目。世界领先的宇宙学和快速射电暴科学将产生与CHIME这个赠款期间。我的研究的另一个主轴是宇宙微波背景（CMB）偏振仪器和分析。通过新的南极望远镜3g（SPT3g）接收器，由我的团队开发和建造的低温读出技术构建，我们将达到地图深度，使我们能够准确地表征小角度尺度B模式功率谱偏振信号。我们正在开发用于卫星平台的仪器，重点是日本主导的LiteBIRD CMB偏振仪。我是我们最近从加拿大航天局收到的两份合同的首席研究员，这两份合同是为了开发、规划加拿大对LiteBird的贡献并计算成本。本基金五年的研究目标是：（1）开创CHIME分析技术和校准策略 a）为了在红移1至2.5处获得重子声振荡的最佳测量，对暗能量施加了新的限制，以及 B）提供最大的快速射电爆发样本，用已知的统一选择将它们编目。为了实现这一目标，我的团队将开发相关器仪器技术，校准，观测策略和数据分析的圆柱数字射电望远镜。（2）开发我们团队的数字读出技术，该技术已经部署在SPT3g上，用于太空，使LiteBIRD卫星CMB偏振计成为可能。分析来自SPT3g的新极化数据。（3）为新一代射电望远镜站开发仪器，以便精确定位FRB。我的团队因推动仪器的进步而赢得了国际声誉，这些仪器使新的宇宙学测量成为可能。该团队包括天文学家、物理学家和工程师。它的部分力量来自于团队成员的种族、社会和性别多样性。我们经常与工业合作伙伴合作，衍生技术已被国际上许多研究人员使用。

The primary focus of my research program is to shed light on the origin, fate, and composition of the universe through end-to-end direct astrophysical measurements. New instruments have been enabled by key technology developed by my group, opening new observational windows on some of the most exciting cosmic epochs. Group members have been key authors for important cosmology results with these instruments. My team co-developed and co-built the Canadian Hydrogen Intensity Mapping Experiment (CHIME), a novel new radio telescope that saw first light in Fall 2017. We have been at the core of the CHIME instrument design and realization, taking responsibility for the GHz digitizers and FPGA-based correlator and guiding the overall project. World leading cosmology and Fast Radio Burst science will be produced with CHIME this grant period. The other primary axis of my research is cosmic microwave background (CMB) polarization instrumentation and analysis. With the new South Pole Telescope 3g (SPT3g) receiver, constructed with cryogenic readout technology developed and built by my team, we will reach map depths that allow us to accurately characterize the small angular scale B-mode power spectrum polarization signal. We are developing our instrumentation for satellite platforms, focusing on the Japanese-led LiteBIRD CMB polarimeter. I am the Principle Investigator for two contracts we recently received from the Canadian Space Agency to develop, plan and cost the Canadian contribution to LiteBIRD. The ambitious research goals for this five year grant period are: (1)Pioneer the analysis techniques and calibration strategies to use CHIME      a) for the best measurement of Baryon Acoustic Oscillations available at redshift 1 to 2.5, placing new constraints on Dark Energy, and      b) to provide the largest sample of Fast Radio Bursts, cataloging them with a known, uniform selection. To achieve this, my team will develop the correlator instrumentation techniques, calibration, observing strategy and data analysis for cylindrical digital radio telescopes. (2)Develop our team's digital readout technology, already deployed on SPT3g, for space, enabling the LiteBIRD satellite CMB polarimeter. Analyze new polarization data from SPT3g. (3)Develop instrumentation for new generation radio telescope stations that will allow precise localization of the FRBs. My group has earned an international reputation for driving advances in instrumentation that enable new cosmology measurements. The team includes astronomers, physicists and engineers. It derives part of its strength from racial, social, and gender diversity of team members. We collaborate frequently with industrial partners and spin-off technology has been used by many researchers internationally.